RAPTOR - I. Time-dependent radiative transfer in arbitrary spacetimes

T. Bronzwaer; J. Davelaar; Z. Younsi; M. Mościbrodzka; H. Falcke; M. Kramer; L. Rezzolla

doi:10.1051/0004-6361/201732149

Home

All issues

Volume 613 (May 2018)

A&A, 613 (2018) A2

Full HTML

Free Access

Table 3

Integrated flux density computed by RAPTOR and BHOSS for the model described in Sect. 4.2.2, as well as the relative error, showing convergence of the output of the two codes.

Pixels	I_{230 GHz, RAPTOR}	I_{230 GHz, BHOSS}	ΔI∕I
128 × 128	2.39467	2.36903	1.07
256 × 256	2.39794	2.38237	0.65
512 × 512	2.39871	2.39133	0.31
1024 × 1024	2.39899	2.39553	0.14
2048 × 2048	2.39898	2.39777	0.050
4096 × 4096	2.39896	2.39881	0.0063

Notes. The last column reports the relative difference between the two codes, which is, Δ I∕I := (I_{230 GHz, RAPTOR} − I_{230 GHz, BHOSS})∕I_{230 GHz, RAPTOR}.

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.